「Longitude」の共起表現(1語右で並び替え)

「Longitude」の共起表現一覧(1語右で並び替え)

Longitude

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Longitude: about 78.533 (78°32'0") W
r use the moon's position to determine their longitude accurately.
The Longitude Act was an Act of Parliament of the United K
ented to Westminster Palace in May 1714, the Longitude Act was passed in July 1714.
Only one packet encodes latitude and longitude, altitude, direction, and speed (full positi
Current location - current latitude, longitude, altitude, direction, and speed of the phone
ricane slowly turned to the north along 83°W Longitude, and it steadily intensified on October 17.
the island where they have to determine the longitude and latitude of the island, create a radio f
graphic position being 24°51'12”-26°13'52” E longitude and 43°55'31”-44°49'32” N latitude.
tion in right ascension, but not in ecliptic longitude and vice versa.
s on a sphere given angular positions (e.g., longitude and latitude).
section with the Meridian of 57 degrees West Longitude and the shoreline of the southwest coast, lo
public lecture, as did Dava Sobel, author of Longitude, and Sir Arnold Wolfendale, the 14th Astrono
translational position (typically latitude, longitude and altitude) over a period of time.
ublished in his lifetime, but left papers on longitude and the moons of Jupiter that were published
irty U-boats, is marked only by latitude and longitude, and has no name by which it will be remembe
Princeton's longitude and latitude coordinates
Lansing's longitude and latitude coordinates
e and North Branches, at approximately 94.1W longitude, and 44.5N latitude.
of Venus with the sun, and thus finding its longitude and latitude, while other stars could at any
situated at 12'41'30" latitude and 74'58'00" longitude and 28m elevated from M.S.L.
West Longitude and is 16 kilometers across.
West Longitude and is 15 kilometers across.
West Longitude and is 18 kilometers across.
West Longitude and is 17 kilometers across.
surface, discovered the Moon's libration in longitude, and published his results in Selenographia,
West Longitude, and is 15.4 kilometers across.
West Longitude, and is 9 kilometers across.
West Longitude, and is ten kilometers across.
cated at 9.8° south latitude and 193.2° west longitude and is 85.9 km in diameter.
W. longitude, and has an area of 4.4 km2.
West Longitude and is approximately 132 kilometres long.
The website provides the best known longitude and latitude (sometimes only accurate to wit
West Longitude and is approximately 20 kilometers across.
West Longitude and is approximately 15 kilometers across.
West Longitude and is approximately 201 kilometers long.
The longitude and latitude of its center are 311.6°
Keokuk's longitude and latitude coordinates in decimal form are
West Longitude and is approximately 311 km across.
he title indicates that specific time, date, longitude, and latitude.
ts name indicate, respectively, the galactic longitude and latitude, and velocity towards Earth in
It reaches 17″ in longitude and 9″ in obliquity.
It established the Board of Longitude and offered a monetary reward (Longitude Pri
ands in the south Pacific that they knew the longitude and latitude.
located at 63.1° North Latitude, 16.9° West Longitude and is 34 kilometers across.
is a transparent circular grid with lines of longitude and latitude that which can overlay a solar
e village is situated at 38 º 27 'N, 6 º 00' longitude and an altitude of 481 m.
It was positioned at 82ºW longitude, and operated by Telesat Canada.
This arctic sea is located at 82° north longitude and 21° west latitude.
It will be positioned at 111° West longitude, and is expected to operate for 15 years.
The 3D position (latitude, longitude and elevation) of each theodolite is known.
in one direction or with similar ecliptical longitude) and to opposition (both sun and moon observ
intersection of the Meridian of 57o30' West Longitude and the southern shoreline
tion of the drop, indicated by the latitude, longitude, and Marsden Square.
orrected so that its pixels are aligned with longitude and latitude lines, and have a narrowly defi
yne hired him as a computer for the board of longitude, and two of his mathematical papers were pre
located at 57.2° North Latitude, 12.0° West Longitude and is 35 kilometers across.
e aircraft's identifier, position (latitude, longitude, and altitude), date and time, flight level,
usually reported at intervals of 10 degrees longitude and are used primarily by airline class airc
he exact time of midday there (an adjunct of longitude), and became for a while the arbiter of time
hin the geographical limit of 78o15'-78o45'E longitude and 11o44'-12o08'N latitude.
hroat Island, Frenchman´s Creek, Shaka Zulu, Longitude, and Wives and Daughters.
Their appearance and longitude are irregular due to a lack of synchonizatio
on, supergalactic latitude and supergalactic longitude are usually denoted by SGB and SGL, respecti
int must be defined from which the angles of longitude are measured.
Their appearance and longitude are irregular due to a lack of synchonizatio
s from the intersection of this latitude and longitude are protected under the provisions of Histor
e 1m-class optical telescopes distributed in longitude around the southern hemisphere in order to p
the highest mean annual temperature at each longitude around the globe.
for the Moon to return to the same ecliptic longitude as the Sun: the synodic month.
The Board of Longitude asked Kendall to copy and develop John Harri
of a series of experiments used to determine longitude at sea.
West Longitude, at the base of the continental slope of Nor
Branchville has a latitude at 31.15 and a longitude at -84.315.
way of enabling mariners to determine their longitude at sea.
onometer for precise clocks designed to find longitude at sea.
es corresponding to 30 degrees difference in longitude, at different latitudes
els a sun-synchronous orbit, passing a given longitude at 10:30 AM local time.
This brought the problem of measuring longitude at sea into sharp focus once more.
allowed navigators to successfully calculate longitude at sea.
solutions were proposed for how to determine longitude at the end of an exploratory sea voyage and
e wide range of estimates of the distance in longitude between Toledo and Rome.
new land at 62° south lattitude and 60° west longitude, but did not land on it.
Longitude, but no Richter Scale magnitude can be asses
r ring, the other on a method of determining longitude by means of lunar eclipses.
The Method of Finding the Longitude by Timekeepers (1794)
atellites and on the mode of determining the longitude by these means (1810)
inclination and the ascending node, the true longitude can tell us the precise direction from the c
alk rate - the rate at which the areocentric longitude changed with each orbit, and the periapsis w
ies and districts for which the latitude and longitude coordinates are included below, may be seen
Latitude and longitude coordinates are provided for many National R
ies and districts for which the latitude and longitude coordinates are included below, may be seen
Register district for which the latitude and longitude coordinates are included below, may be seen
ies and districts for which the latitude and longitude coordinates are included below, may be seen
gister properties for which the latitude and longitude coordinates are included below, may be seen
ies and districts for which the latitude and longitude coordinates are included below, may be seen
Latitude and longitude coordinates are provided for many National R
above sea level and is located at latitude - longitude coordinates of N 36.829028
ies and districts for which the latitude and longitude coordinates are included below may be seen i
Turtle Mound is located at the latitude and longitude coordinates of N 28.93082 and W -80.827
l properties and districts with latitude and longitude coordinates in the table below.
ricts (at least for all showing latitude and longitude coordinates below) may be seen in a Google m
imal place of one second of the latitude and longitude coordinates).
The latitude longitude cordinates for Christopher Nagar is 8°11'14"
nd RootsMagic are supported for latitude and longitude data.
A longitude describes the location of a place on Earth e
o obtain a location could input latitude and longitude details to see how far away other online use
t this would eventually solve the problem of longitude determination for ocean navigators.
ne chronometer, thereby allowing for precise longitude determination while at sea.
He believed he could improve the accuracy of longitude determination, particularly at sea, by obser
he meridian of Jerusalem, corresponding to a longitude difference of 8°55'.
rt to redetermine with greater precision the longitude difference between London and Paris.
etween England and France - this would allow longitude differences to be measured very accurately,
le can be expressed in terms of latitude and longitude differences dlat,dlong, using only cosines,
ed at the crossing of Latitude N 23 -50` and Longitude E 91-17`, covering 3 km² during that period.
this region is divided into 12 signs of 30° longitude each.
Supports GEDCOM 5.5.1 draft's Latitude and Longitude extensions.
Character pairs encode longitude first, and then latitude.
stward to its intersection with the 21° east longitude, follows this degree of longitude northward
d Arnold were granted awards by the Board of Longitude for their improvements to chronometers; Earn
ension and declination are like latitude and longitude for astronomy).
had been working on the problem of measuring longitude for a long time.
Mary Croarken (2002), "Providing Longitude for All", Journal of Maritime Research (Nati
useful at sea; particularly for deducing the longitude from lunar distance, and the latitude from t
in latitude from 41° 20' to 42° 40' N and in longitude from 109° 50' to 111° 25' E.
e 9-1-1 center is provided with latitude and longitude from the radio's GPS receiver.
s in latitude from 27° 50'-29° 16' N, and in longitude from 103° 36'-105° 20' E, stretching 153 kil
teroids and comets and on the measurement of longitude, improving the accuracy of the Connaissance
ed its orbit to within 2 arcminutes error in longitude in his geoheliocentric model when Kepler had
located at 6° north latitude and 355.5° west longitude in the Oxia Palus quadrangle.
To determine longitude in navigation, Werner proposed determining t
ts designated orbital slot is 74 degree East longitude in the Geostationary Orbit.
e observatory was moved closer to the 82.5°E longitude in Mirzapur in Uttar Pradesh.
The satellite was positioned at 4° W longitude in the geo-stationary orbit.
It became operational at 74° West longitude in the geostationary orbit and replaced SBS-
Longitude incorrectly marked as East rather than West.
The longitude is -97.2W.
The longitude is -80.375W.
In this case, the longitude is also called the right ascension of the as
The longitude is -93.855W).
The longitude is -80.976W.
The longitude is -81.076W.
The longitude is -88.13W.
The longitude is -89.49W.
The longitude is -73.945W.
latitude of this place is 29°40'33"N and the longitude is 80°16'20"E.
The zero point for supergalactic longitude is defined by the intersection of this plane
Its latitude of is 26.784N and its longitude is -80.037W.
In astrodynamics true longitude is the longitude at which an orbiting body c
Greenough's latitude is at 31.317 and its longitude is at -84.102.
Its latitude is 41.2833/41º16'60 N and its longitude is 1.36667/01º22'0 E. The population in 2003
Flint's latitude is at 31.317 and its longitude is at -84.179.
latitude of Creighton is 40.587N, while the longitude is -79.778W.
Thus, the area between two meridians of longitude is a lune.
The latitude of Breed is 45.073N and the longitude is -88.424W.
The longitude is-89.656W.
of Mars at 48.6° south latitude and 26° west longitude, It is 129 km in diameter and was named afte
ree southern latitude and 76 degrees western longitude, just between the Martian equator and the Va
oper River was on the corner of East Bay and Longitude Lane.
the region along the later-proposed 70º east longitude line was proposed by the Empire of Japan in
d border and from east of the 78 degree west longitude line to just west of Chambersburg, PA.
cause it lies as far as 30° east of the 180° longitude line), and thus the first part of the planet
y Mouse-shaped globe containing latitude and longitude lines, with the property's name presented in
e, the stars shift eastwards (increase their longitude) measured with respect to the equinoxes - in
ing one degree of latitude and one degree of longitude, named according to their south western corn
es were 3°34' north latitude and 56°30' east longitude, near the edge of the Mare Fecunditatis ("Se
conjunctions in right ascension and ecliptic longitude need not to take place on the same date.
day when the Sun is exactly at the celestial longitude of 120°.
day when the Sun is exactly at the celestial longitude of 240°.
feet) at a latitude of 7.65°N (7°39'0"N) and longitude of 124.45°E (124°27'0"E).
e unexplained fluctuation in the Moon's mean longitude of the order of 10 arcseconds.
ard Time Zone at a latitude of 36.248N and a longitude of -82.545W.
me at Greenwich by a difference equal to the longitude of the fictitious mean Sun used for defining
and Longitude of 089º56.456.
day when the Sun is exactly at the celestial longitude of 195°.
ts was the determination of the latitude and longitude of Washington, D.C. in 1846.
day when the Sun is exactly at the celestial longitude of 285°.
day when the Sun is exactly at the celestial longitude of 30°.
pradesh with latitude of 28 degree north and longitude of 95 degree east.
semi-major axis, eccentricity, inclination, longitude of periastron, time of periastron, maximum t
is longitude of orbit's periapsis,
day when the Sun is exactly at the celestial longitude of 150°.
en DnaG and DnaB is necessary to control the longitude of Okazaki fragments on the lagging strand.
fined by two parameters, Inclination (i) and Longitude of the ascending node (Ω).
of not implying knowledge of the historical longitude of continents, which is difficult to determi
day when the Sun is exactly at the celestial longitude of 180°.
eostationary orbit, and will be located at a longitude of 61.5° West, from where it is intended to
Bombay, and Canton; as also the Latitude and Longitude of Point de Galle and the Friar's Hood."
longitude of the perihelion: 159.079 degree
ged in the determination of the latitude and longitude of prominent capes, bays, etc., and of the m
longitude of ascending node: 218.993 degree
longitude of the ascending node: 41.07311 deg
stars, so as to find out the so-much desired longitude of places for the perfecting the art of navi
ane of reference are the inclination and the longitude of the ascending node.
1 was positioned in geostationary orbit at a longitude of 104° West for testing and on-orbit storag
Longitude of the ascending node: 92.24656 degree (equi
It will be positioned at a longitude of 1° West.
It has a Latitude of 42° 57' 0 North,a Longitude of 4° 5' 60 West, and an Altitude of 3481 fe
It begins when the Sun reaches the celestial longitude of 45° and ends when it reaches the longitud

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